Setup environment
ssh pslogin
ssh psana
cd <your-directory>
sit_setup
Examples for xpp50312
Pedestals
In this section we show how to get CSPad2x2 pedestals using psana for "dark" run.
For this example we create the configuration file ana-xpp50312/psana-xpp50312-r0082-pedestals.cfg
:
[psana] files = /reg/d/ana01/xpp/xpp50312/xtc/e178-r0082-s04-c00.xtc modules = cspad_mod.CsPad2x2Pedestals [cspad_mod.CsPad2x2Pedestals] #source = DetInfo(:Cspad2x2) source = DetInfo(XppGon.0:Cspad2x2.0) output = cspad-pedestals-ave-xpp50312-r0082.dat noise = cspad-pedestals-rms-xpp50312-r0082.dat
Run psana with this configuration file:
psana -c ana-xpp50312/psana-xpp50312-r0082-pedestals.cfg
In a few seconds this job produces two text files with averaged pedestals and rms values as one-dimensional (143560) array for CSPad2x2. Actual shape of these arrays is assumed to be (185,388,2).
Using, for example, a simple python script these files may be plotted
./PlotCSPad2x2ArrayFromFile.py cspad-pedestals-ave-xpp50312-r0082.dat 700 1400
./PlotCSPad2x2ArrayFromFile.py cspad-pedestals-rms-xpp50312-r0082.dat 0 20
Averaged pedestals:
RMS of pedestals:
Calibration
By default psana assumes that all calibration files are located in the pre-defined directory
/reg/d/psdm/<INSTRUMENT>/<experiment>/calib/
as explained in Locating calibration files. However, for analysis it may be convenient to re-define the calibration directory through the psana parameters. In order to fulfill the naming conventions we have to create a tree of the calibration sub-directories somewhere in local user's space, for example:
ana-xpp50312/calib/CsPad2x2::CalibV1/XppGon.0:Cspad2x2.0/pixel_gain/ pixel_status/ pedestals/ common_mode/
and populate them with all necessary for analysis files. In particular, for pedestals we can use:
cp cspad-pedestals-ave-xpp50312-r0082.dat ana-xpp50312/calib/CsPad2x2::CalibV1/XppGon.0:Cspad2x2.0/pedestals/82-end.data
Another file for common mode correction common_mode/0-end.data
usually looks like
1 50 10
The files for pixel_status
and pixel_gain
have the same structure like for pedestals
and can be supplied, if necessary, depending and based on analysis.
Analysis
For this example we create the configuration file ana-xpp50312/psana-xpp50312-r0092.cfg
:
[psana] files = /reg/d/ana01/xpp/xpp50312/xtc/e178-r0092-s04-c00.xtc experiment = xpp50312 calib-dir = ana-xpp50312/calib events = 10 modules = cspad_mod.CsPadCalib CSPadPixCoords.CSPad2x2ImageProducer CSPadPixCoords.SaveImageInFile [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated doPedestals = yes doPixelStatus = no doCommonMode = yes doPixelGain = no [CSPadPixCoords.CSPad2x2ImageProducer] source = DetInfo(:Cspad2x2) inkey = calibrated outimgkey = Image tiltIsApplied = true print_bits = 15 [CSPadPixCoords.SaveImageInFile] source = DetInfo(:Cspad2x2) key = Image fname = cspad2x2 eventSave = 5 #saveAll = true
This configuration file provides parameters for psana and three modules.
So far we setup calibration files for cspad_mod.CsPadCalib
module for pedestal subtraction and common mode correction. Module CSPadPixCoords.CSPad2x2ImageProducer
produces the CSPad2x2 image and saves it in the event. Module SaveImageInFile
saves indicated image(s) in the file(s).
Run psana with this configuration file:
psana -c ana-xpp50312/psana-xpp50312-r0092.cfg
Plot obtained text file with an image:
./PlotCameraImageFromFile.py cspad2x2-r0092-2012-07-20-154000.855680176.txt -20 120
Playing with doPedestals
and doCommonMode
parameters, we could get different images.
Raw data without any correction:
Pedestals subtracted:
Pedestals subtracted and common mode corrected:
Examples for meca6113
Pedestals
Configuration file for dark run processing (assuming that meca6113-r0018 is a dark run...) psana-meca6113-r0018-cspad2x2-pedestals.cfg:
# File: psana-meca6113-r0018-cspad2x2-pedestals.cfg [psana] files = /reg/d/psdm/mec/meca6113/xtc/e332-r0018-s03-c00.xtc modules = cspad_mod.CsPad2x2Pedestals:1 \ cspad_mod.CsPad2x2Pedestals:2 \ cspad_mod.CsPad2x2Pedestals:3 [cspad_mod.CsPad2x2Pedestals:1] source = DetInfo(MecTargetChamber.0:Cspad2x2.1) output = pedestals-ave-meca6113-r0018-Cspad2x2.1.dat noise = pedestals-rms-meca6113-r0018-Cspad2x2.1.dat [cspad_mod.CsPad2x2Pedestals:2] source = DetInfo(MecTargetChamber.0:Cspad2x2.2) output = pedestals-ave-meca6113-r0018-Cspad2x2.2.dat noise = pedestals-rms-meca6113-r0018-Cspad2x2.2.dat [cspad_mod.CsPad2x2Pedestals:3] source = DetInfo(MecTargetChamber.0:Cspad2x2.3) output = pedestals-ave-meca6113-r0018-Cspad2x2.3.dat noise = pedestals-rms-meca6113-r0018-Cspad2x2.3.dat
To produce files with pedestals use command:
psana -c psana-meca6113-r0018-cspad2x2-pedestals.cfg
which produces 6 files with average and rms values for 3 detectors:
pedestals-ave-meca6113-r0018-Cspad2x2.1.dat pedestals-ave-meca6113-r0018-Cspad2x2.2.dat pedestals-ave-meca6113-r0018-Cspad2x2.3.dat pedestals-rms-meca6113-r0018-Cspad2x2.1.dat pedestals-rms-meca6113-r0018-Cspad2x2.2.dat pedestals-rms-meca6113-r0018-Cspad2x2.3.dat
Example of pedestal-image and spectral plots for 3 detectors, respectively:
Calibration
Default calibration in psana will be done if files are located in right place. So, they were deployed as:
cp pedestals-ave-meca6113-r0018-Cspad2x2.1.dat /reg/d/psdm/mec/meca6113/calib/CsPad2x2::CalibV1/MecTargetChamber.0:Cspad2x2.1/pedestals/18-end.data cp pedestals-ave-meca6113-r0018-Cspad2x2.2.dat /reg/d/psdm/mec/meca6113/calib/CsPad2x2::CalibV1/MecTargetChamber.0:Cspad2x2.2/pedestals/18-end.data cp pedestals-ave-meca6113-r0018-Cspad2x2.3.dat /reg/d/psdm/mec/meca6113/calib/CsPad2x2::CalibV1/MecTargetChamber.0:Cspad2x2.3/pedestals/18-end.data
Create images in tiff format
Configuration file for psana psana-meca6113-r0028-cspad2x2-tiff.cfg:
# File: psana-meca6113-r0028-cspad2x2-tiff.cfg # # To run this script use command: # % psana -c psana-meca6113-r0028-cspad2x2-tiff.cfg # # Also useful command: # % psana -m EventKeys -n 10 /reg/d/psdm/mec/meca6113/xtc/e332-r0028-s03-c00.xtc # [psana] files = /reg/d/psdm/mec/meca6113/xtc/e332-r0028-s03-c00.xtc #calib-dir = ./calib # Default calibration directory: # calib-dir = /reg/d/psdm/mec/meca6113/calib modules = cspad_mod.CsPadCalib:1 \ cspad_mod.CsPadCalib:2 \ cspad_mod.CsPadCalib:3 \ CSPadPixCoords.CSPad2x2ImageProducer:1 \ CSPadPixCoords.CSPad2x2ImageProducer:2 \ CSPadPixCoords.CSPad2x2ImageProducer:3 \ ImgAlgos.ImgSaveInFile:1 \ ImgAlgos.ImgSaveInFile:2 \ ImgAlgos.ImgSaveInFile:3 # events = 5 [cspad_mod.CsPadCalib:1] source = DetInfo(MecTargetChamber.0:Cspad2x2.1) inputKey = outputKey = calibrated_arr1 doPedestals = yes doPixelStatus = no doCommonMode = no [cspad_mod.CsPadCalib:2] source = DetInfo(MecTargetChamber.0:Cspad2x2.2) inputKey = outputKey = calibrated_arr2 doPedestals = yes doPixelStatus = no doCommonMode = no [cspad_mod.CsPadCalib:3] source = DetInfo(MecTargetChamber.0:Cspad2x2.3) inputKey = outputKey = calibrated_arr3 doPedestals = yes doPixelStatus = no doCommonMode = no [CSPadPixCoords.CSPad2x2ImageProducer:1] calibDir = /reg/d/psdm/mec/meca6113/calib typeGroupName = CsPad2x2::CalibV1 source = DetInfo(MecTargetChamber.0:Cspad2x2.1) inkey = calibrated_arr1 outimgkey = Image tiltIsApplied = true useWidePixCenter = false print_bits = 15 [CSPadPixCoords.CSPad2x2ImageProducer:2] calibDir = /reg/d/psdm/mec/meca6113/calib typeGroupName = CsPad2x2::CalibV1 source = DetInfo(MecTargetChamber.0:Cspad2x2.2) inkey = calibrated_arr2 outimgkey = Image tiltIsApplied = true useWidePixCenter = false print_bits = 15 [CSPadPixCoords.CSPad2x2ImageProducer:3] calibDir = /reg/d/psdm/mec/meca6113/calib typeGroupName = CsPad2x2::CalibV1 source = DetInfo(MecTargetChamber.0:Cspad2x2.3) inkey = calibrated_arr3 outimgkey = Image tiltIsApplied = true useWidePixCenter = false print_bits = 15 [ImgAlgos.ImgSaveInFile:1] source = DetInfo(MecTargetChamber.0:Cspad2x2.1) key = Image fname = cspad2x2.1 #ftype = txt ftype = tiff saveAll = true print_bits = 3 #eventSave = 5 [ImgAlgos.ImgSaveInFile:2] source = DetInfo(MecTargetChamber.0:Cspad2x2.2) key = Image fname = cspad2x2.2 #ftype = txt ftype = tiff saveAll = true print_bits = 3 #eventSave = 5 [ImgAlgos.ImgSaveInFile:3] source = DetInfo(MecTargetChamber.0:Cspad2x2.3) key = Image fname = cspad2x2.3 #ftype = txt ftype = tiff saveAll = true print_bits = 3 #eventSave = 5
To produce files with images in tiff format use command:
psana -c psana-meca6113-r0028-cspad2x2-tiff.cfg
New files will be produced with names containing time stamp:
cspad2x2.1-r0028-20131013-155538.754093925.tiff cspad2x2.2-r0028-20131013-155538.754093925.tiff cspad2x2.3-r0028-20131013-155538.754093925.tiff
Example of image and spectral plots for 3 detectors, respectively:
Examples for meca1113
Get latest version of packages and run psana
On 6 p.m. 2013-11-13 all recent code changes are included in release ana-0.10.5 (seen in directory $SIT_RELDIR).
To run psana use commands:
ssh -Y psana cd <your-favorite-directory> sit_setup cp <path-to-where-it-is-located>/psana-meca1113-r0376-cspad-cspad2x2-tiff.cfg . psana -c psana-meca1113-r0376-cspad-cspad2x2-tiff.cfg
or run xtcexplorer:
xtcexplorer /reg/d/psdm/mec/meca1113/xtc/e356-r0376-s03-c00.xtc
Pedestals and bad pixels
The configuration file for psana psana-meca1113-r0045-cspad-cspad2x2-dark-hotpix.cfg can be used to produce calibration files with pedestals (dark rate) and mask of bad pixels:
# Run this script: # psana -c psana-meca1113-r0045-cspad-cspad2x2-dark-hotpix.cfg [psana] # Default calibration directory: # calib-dir = /reg/d/psdm/mec/meca1113/calib files = exp=meca1113:run=45 events = 400 #skip-events = 0 modules = CSPadPixCoords.CSPadNDArrProducer \ CSPadPixCoords.CSPad2x2NDArrProducer:1 \ CSPadPixCoords.CSPad2x2NDArrProducer:2 \ CSPadPixCoords.CSPad2x2NDArrProducer:3 \ CSPadPixCoords.CSPad2x2NDArrProducer:4 \ ImgAlgos.NDArrAverage \ ImgAlgos.NDArrAverage:1 \ ImgAlgos.NDArrAverage:2 \ ImgAlgos.NDArrAverage:3 \ ImgAlgos.NDArrAverage:4 \ ImgAlgos.Tahometer [CSPadPixCoords.CSPadNDArrProducer] source = MecTargetChamber.0:Cspad.0 inkey = outkey = cspad_ndarr outtype = int16 is_fullsize = yes print_bits = 3 [CSPadPixCoords.CSPad2x2NDArrProducer:1] source = MecTargetChamber.0:Cspad2x2.1 inkey = outkey = cspad2x2.1_ndarr outtype = int16 print_bits = 3 [CSPadPixCoords.CSPad2x2NDArrProducer:2] source = MecTargetChamber.0:Cspad2x2.2 inkey = outkey = cspad2x2.2_ndarr outtype = int16 print_bits = 3 [CSPadPixCoords.CSPad2x2NDArrProducer:3] source = MecTargetChamber.0:Cspad2x2.3 inkey = outkey = cspad2x2.3_ndarr outtype = int16 print_bits = 3 [CSPadPixCoords.CSPad2x2NDArrProducer:4] source = MecTargetChamber.0:Cspad2x2.4 inkey = outkey = cspad2x2.4_ndarr outtype = int16 print_bits = 3 [ImgAlgos.NDArrAverage] source = MecTargetChamber.0:Cspad.0 key = cspad_ndarr avefile = cspad.0-ave rmsfile = cspad.0-rms maskfile = cspad.0-msk hotpixfile = cspad.0-hot thr_rms_ADU = 10 thr_min_ADU = 2 thr_max_ADU = 65000 print_bits = 93 [ImgAlgos.NDArrAverage:1] source = MecTargetChamber.0:Cspad2x2.1 key = cspad2x2.1_ndarr avefile = cspad2x2.1-ave rmsfile = cspad2x2.1-rms maskfile = cspad2x2.1-msk hotpixfile = cspad2x2.1-hot #evts_stage1 = 100 #gate_width1 = 100. thr_rms_ADU = 10 thr_min_ADU = 2 thr_max_ADU = 65000 print_bits = 93 [ImgAlgos.NDArrAverage:2] source = MecTargetChamber.0:Cspad2x2.2 key = cspad2x2.2_ndarr avefile = cspad2x2.2-ave rmsfile = cspad2x2.2-rms maskfile = cspad2x2.2-msk hotpixfile = cspad2x2.2-hot #evts_stage1 = 100 #gate_width1 = 100. thr_rms_ADU = 10 thr_min_ADU = 2 thr_max_ADU = 65000 print_bits = 93 [ImgAlgos.NDArrAverage:3] source = MecTargetChamber.0:Cspad2x2.3 key = cspad2x2.3_ndarr avefile = cspad2x2.3-ave rmsfile = cspad2x2.3-rms maskfile = cspad2x2.3-msk hotpixfile = cspad2x2.3-hot #evts_stage1 = 100 #gate_width1 = 100. thr_rms_ADU = 10 thr_min_ADU = 2 thr_max_ADU = 65000 print_bits = 93 [ImgAlgos.NDArrAverage:4] source = MecTargetChamber.0:Cspad2x2.4 key = cspad2x2.4_ndarr avefile = cspad2x2.4-ave rmsfile = cspad2x2.4-rms maskfile = cspad2x2.4-msk hotpixfile = cspad2x2.4-hot #evts_stage1 = 100 #gate_width1 = 100. thr_rms_ADU = 10 thr_min_ADU = 2 thr_max_ADU = 65000 print_bits = 93 [ImgAlgos.Tahometer] dn = 100 print_bits = 7
This script
- runs through 400 events of the xtc file
exp=meca1113:run=45
, uses CSPadNDArrProducer and CSPad2x2NDArrProducer modules to get cspad and four cspad2x2 data and put them as universal
ndarray<T,3>
objects in psana event store,uses NDArrAverage module to evaluate and save in file average, rms, mask, and hot pixel map for all array elements:
cspad.0-ave-meca1113-r0045.dat cspad.0-hot-meca1113-r0045.dat cspad.0-msk-meca1113-r0045.dat cspad.0-rms-meca1113-r0045.dat cspad2x2.1-ave-meca1113-r0045.dat cspad2x2.1-hot-meca1113-r0045.dat cspad2x2.1-msk-meca1113-r0045.dat cspad2x2.1-rms-meca1113-r0045.dat cspad2x2.2-ave-meca1113-r0045.dat cspad2x2.2-hot-meca1113-r0045.dat cspad2x2.2-msk-meca1113-r0045.dat cspad2x2.2-rms-meca1113-r0045.dat cspad2x2.3-ave-meca1113-r0045.dat cspad2x2.3-hot-meca1113-r0045.dat cspad2x2.3-msk-meca1113-r0045.dat cspad2x2.3-rms-meca1113-r0045.dat cspad2x2.4-ave-meca1113-r0045.dat cspad2x2.4-hot-meca1113-r0045.dat cspad2x2.4-msk-meca1113-r0045.dat cspad2x2.4-rms-meca1113-r0045.dat
NDArrAverage module has a bunch of parameters which depend on particular detector/experiments and need to be adjusted looking at spectra of average and rms values from these files. For example averaged image and spectrum and rms spectrum of pixel intensities for
cspad2x2.1-ave-meca1113-r0045.dat and cspad2x2.1-rms-meca1113-r0045.dat
are shown in plots:
These spectra allow to use confidently parameters like
thr_rms_ADU = 10
thr_min_ADU = 2
thr_max_ADU = 65000
Files with mask and hot pixel map contain opposite meaning of 0/1 for bad/good pixels:
Calibration
Default calibration in psana will be done if files are located in right place. So, they were deployed as:
cp cspad.0-ave-meca1113-r0045.dat /reg/d/psdm/mec/meca1113/calib/CsPad::CalibV1/MecTargetChamber.0:Cspad.0/pedestals/45-end.data cp cspad2x2.1-ave-meca1113-r0045.dat /reg/d/psdm/mec/meca1113/calib/CsPad2x2::CalibV1/MecTargetChamber.0:Cspad2x2.1/pedestals/45-end.data cp cspad2x2.2-ave-meca1113-r0045.dat /reg/d/psdm/mec/meca1113/calib/CsPad2x2::CalibV1/MecTargetChamber.0:Cspad2x2.2/pedestals/45-end.data ... cp cspad.0-hot-meca1113-r0045.dat /reg/d/psdm/mec/meca1113/calib/CsPad::CalibV1/MecTargetChamber.0:Cspad.0/pixel_status/45-end.data cp cspad2x2.1-hot-meca1113-r0045.dat /reg/d/psdm/mec/meca1113/calib/CsPad2x2::CalibV1/MecTargetChamber.0:Cspad2x2.1/pixel_status/45-end.data ...
Create images in tiff format
Configuration file for psana psana-meca1113-r0376-cspad-cspad2x2-conv-tiff.cfg
# Run this script: # psana -c psana-meca1113-r0376-cspad-cspad2x2-conv-tiff.cfg # # Useful commands: # psana -m EventKeys -n 5 exp=meca1113:run=376 # or # psana -m EventKeys -n 5 /reg/d/psdm/mec/meca1113/xtc/e356-r0376-s03-c00.xtc [psana] # Default calibration directory: # calib-dir = /reg/d/psdm/mec/meca1113/calib files = exp=meca1113:run=376 events = 5 #skip-events = 0 modules = cspad_mod.CsPadCalib \ CSPadPixCoords.CSPadImageProducer:0 \ CSPadPixCoords.CSPad2x2ImageProducer:1 \ CSPadPixCoords.CSPad2x2ImageProducer:2 \ CSPadPixCoords.CSPad2x2ImageProducer:3 \ CSPadPixCoords.CSPad2x2ImageProducer:4 \ pyimgalgos.image_crop:0 \ pyimgalgos.image_save_in_file:0 \ pyimgalgos.image_save_in_file:1 \ pyimgalgos.image_save_in_file:2 \ pyimgalgos.image_save_in_file:3 \ pyimgalgos.image_save_in_file:4 \ ImgAlgos.Tahometer # Calibrate all CSPAD and CSPAD2x2 [cspad_mod.CsPadCalib] inputKey = outputKey = calibrated_arr doPedestals = yes doPixelStatus = yes doCommonMode = yes [CSPadPixCoords.CSPadImageProducer:0] #calibDir = /reg/d/psdm/mec/meca1113/calib #typeGroupName = CsPad::CalibV1 source = DetInfo(MecTargetChamber.0:Cspad.0) key = calibrated_arr imgkey = image0 tiltIsApplied = false print_bits = 3 [CSPadPixCoords.CSPad2x2ImageProducer:1] #calibDir = /reg/d/psdm/mec/meca1113/calib #typeGroupName = CsPad2x2::CalibV1 source = DetInfo(MecTargetChamber.0:Cspad2x2.1) inkey = calibrated_arr outimgkey = image1 tiltIsApplied = true useWidePixCenter = false print_bits = 3 [CSPadPixCoords.CSPad2x2ImageProducer:2] #calibDir = /reg/d/psdm/mec/meca1113/calib #typeGroupName = CsPad2x2::CalibV1 source = DetInfo(MecTargetChamber.0:Cspad2x2.2) inkey = calibrated_arr outimgkey = image2 tiltIsApplied = true useWidePixCenter = false print_bits = 3 [CSPadPixCoords.CSPad2x2ImageProducer:3] #calibDir = /reg/d/psdm/mec/meca1113/calib #typeGroupName = CsPad2x2::CalibV1 source = DetInfo(MecTargetChamber.0:Cspad2x2.3) inkey = calibrated_arr outimgkey = image3 tiltIsApplied = false useWidePixCenter = false print_bits = 3 [CSPadPixCoords.CSPad2x2ImageProducer:4] #calibDir = /reg/d/psdm/mec/meca1113/calib #typeGroupName = CsPad2x2::CalibV1 source = DetInfo(MecTargetChamber.0:Cspad2x2.4) inkey = calibrated_arr outimgkey = image4 tiltIsApplied = true useWidePixCenter = false print_bits = 3 [pyimgalgos.image_crop:0] source = DetInfo(MecTargetChamber.0:Cspad.0) key_in = image0 key_out = image0_cropped rowmin = 70 rowmax = 900 colmin = 0 colmax = 825 print_bits = 255 [pyimgalgos.image_save_in_file:0] source = DetInfo(MecTargetChamber.0:Cspad.0) key_in = image0_cropped ofname = cspad.0.tiff print_bits = 5 [pyimgalgos.image_save_in_file:1] source = DetInfo(MecTargetChamber.0:Cspad2x2.1) key_in = image1 ofname = cspad2x2.1.tiff print_bits = 5 [pyimgalgos.image_save_in_file:2] source = DetInfo(MecTargetChamber.0:Cspad2x2.2) key_in = image2 ofname = cspad2x2.2.tiff print_bits = 5 [pyimgalgos.image_save_in_file:3] source = DetInfo(MecTargetChamber.0:Cspad2x2.3) key_in = image3 ofname = cspad2x2.3.tiff print_bits = 5 [pyimgalgos.image_save_in_file:4] source = DetInfo(MecTargetChamber.0:Cspad2x2.4) key_in = image4 ofname = cspad2x2.4.tiff print_bits = 5 [ImgAlgos.Tahometer] dn = 100 print_bits = 7
Command:
% psana -c psana-meca1113-r0376-cspad-cspad2x2-tiff.cfg
or for other runs:
% psana -c psana-meca1113-r0376-cspad-cspad2x2-tiff.cfg exp=meca1113:run=378
will run over 5 events from xtc files, applys intensity correction for all CSPAD detectors (if calibration files are provided), produces images and save images for one CSPAD and four CSPAD2x2 detectors in 16-bit tiff files, with names like
cspad.0-r0376-e0000000#-20131110-101607.736131763.tiff
cspad2x2.#-r0376-e0000000#-20131110-101546.244253562.tiff
...
Examples for mecb3114
Experiment mecb3114 use different detectors in different runs. Not all of them collected data in each run. Then it make sense to produce tiff files for separate detectors.
Configuration file for MecTargetChamber.0:Cspad2x2: psana-mecb3114-r0008-cspad2x2-tiff.cfg
Configuration file for MecTargetChamber.0:Cspad.0: psana-mecb3114-r0323-cspad-tiff.cfg
Command to run:
% psana -m <file-name>.cfg exp=mecb3114:run=376
Examples for meci0114
Andreas Schropp needs to access cspad image in his custom psana module.
On 2014-03-21 Module ImgAlgos::ExampleDumpImg is add as an example.
Get and run this example in current release
For releases ≤ ana-0.10.14 the updated version of code can be compiled and run from local release directory;
ssh -Y psana cd <your-favorite-directory> kinit <next 6 lines can be copied and pasted> newrel ana-0.10.14 my-release-dir; cd my-release-dir; sit_setup; addpkg ImgAlgos HEAD; addpkg CSPadPixCoords HEAD; scons -j 8; <wait a few minutes until it is compiled> <pick-up *.cfg files and run them> psana -c psana-meci0114-r0050-exampleimgdump-cspadcalib.cfg psana -c psana-meci0114-r0050-exampleimgdump-ndarrcalib.cfg
These example print too much, but this is an intentional example. Level of verbosity can be controlled by the print_bits
parameter for each module.
Configuration files
- psana-meci0114-r0050-exampleimgdump-cspadcalib.cfg - use sequence of CsPadCalib, CSPadImageProducer, and ExampleDumpImg modules
works with int16_t data on all stages until ExampleDumpImg
- psana-meci0114-r0050-exampleimgdump-ndarrcalib.cfg - use sequence of CSPadNDArrProducer, NDArrCalib, CSPadImageProducer, and ExampleDumpImg modules
CSPadNDArrProducer - creates ndarray<const T,3> for a few generic data types,
NDArrCalib - may apply more corrections than CsPadCalib.
ExampleDumpImg - also may process a few data types such as int16_t, int, float, and double.
Other option to save image in 16-bit tiff files
Psana can use python modules. A few modules in package pyimgalgos were recently developed to process CSPAD data.
Psana Module Catalog - Package pyimgalgos
Psana Module Examples - Examples for Package pyimgalgos
In particular, module pyimgalgos.image_save_in_file
may save image in 16-bit tiff files.
Display tiff image
To display image from tiff file use display
command:
display <file-name>.tiff
then
- left mouse click on image
- click on "Enhance" button
- click on "Equalize" button
Other option - use ImageJ
command:
/reg/common/package/imagej/ImageJ <file-name>.tiff
Check tiff file
To check tiff file format one may use command:
% identify -verbose <file-name>.tiff
which prints information about tiff file structure. For example,
% identify -verbose cspad.0-r0376-e00000001-20131110-101546.244253562.tiff Image: cspad.0-r0376-e00000001-20131110-101546.244253562.tiff Format: TIFF (Tagged Image File Format) Class: PseudoClass Geometry: 1750x1750 Type: Grayscale Endianess: MSB Colorspace: Gray Channel depth: Gray: 16-bits Channel statistics: Gray: Min: 0 (0) Max: 16383 (0.249989) Mean: 1023.37 (0.0156156) Standard deviation: 2132.77 (0.0325439) Colors: 65536 ...
Convert uint16 tiff to int16 tiff
Eric Galtier found the way to change file format record for tiff file using convert command:
convert input_file.tiff -define quantum:format=signed output_file.tiff
Other option for floating point conversion: -define quantum:format=floating-point
Examples for cxi86415
This test is done by request
Loh, Ne-Te writes:
> On a separate note, the online monitoring software (hummingbird, by Benedikt and Filipe) will need py+psana. However, the default psana calibrations/corrections for the 140k back detector seems wonky. You might recall that there was a teleconference where Veitâ's student (Yi-Tien) discusses how the 0-photon peak had a largish negative ADU, despite turning on common mode correction and dark subtraction (psana's implementation). Would you and your team be able to take a look at these as well? If it's a quick fix, then the online monitoring group will have a much easier time (e.g. they won't have to separately do common mode subtraction).
Standard configuration file
Use psana configuration file psana-cxidg3-cspad2x2-NDArrAverage.cfg (download), which can be executed by command:
sit_setup psana -c psana-cxidg3-cspad2x2-NDArrAverage.cfg exp=cxi86415:run=7
This job produces 3 files with cspad2x2 shaped arrays for averaged, rms, and maximal intensities.
These arrays can be plotted by the command
plims cspad2x2-ndarr-ave-cxi86415-r0007.dat
Results for runs 7, 62, and 83 are shown on plots:
These plots show that the dark level is consistent with zero and does not indicate on any offset.
Loh's configuration file
Use configuration file from Loh's e-mail orig.cfg (download)
with minor modifications
- add psana parameters in the header, add list of modules
- remove
typeGroupname = CsPad:CalibV1 from
[CSPadPixCoords.CSPad2x2ImageProducer:2]
- add module
ImgAlgos.ImgSaveInFile:2
just in order to save image:
[psana] files = exp=cxi86415:run=64 events = 10 modules = CSPadPixCoords.CSPad2x2NDArrProducer:2 \ ImgAlgos.NDArrCalib:2 \ CSPadPixCoords.CSPad2x2ImageProducer:2 \ ImgAlgos.ImgSaveInFile:2 <code from e-mail is here> [ImgAlgos.ImgSaveInFile:2] source = DetInfo(CxiDg3.0:Cspad2x2.0) key = reconstructed fname = img-cspad2x2-dg3 ftype = txt #saveAll = true print_bits = 3 eventSave = 9
Run it with command:
psana -c orig.cfg
which produces file with image for event #9, which can be viewed as
plims img-cspad2x2-dg3-cxi86415-r0064-e00000009-20150308-162942.145136207.txt
ang brings us an image: - the same image, but spectrum is shown in the range (-100, 100) ADU. This event looks good.
Event #36: looks like left-side sensor is not corrected for common mode fluctuation...
In stead of default common_mode parameters (1,25,25,100) let us try (1,50,10,100) in the file
/reg/d/psdm/CXI/cxi86415/calib/CsPad2x2::CalibV1/CxiDg3.0:Cspad2x2.0/common_mode/9-end.data
The same image looks better now:
Recommendation: try to play with common mode parameters.
References
NDArrAverage module